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Title: Absorption of gravitational waves from distant sources

Abstract

The rate of gravitational wave absorption by inverse bremsstrahlung is calculated. It increases with decreasing frequency ν as ν–3. Nevertheless, because of the near cancellation of absorption by stimulated emission, the ionized gas in galaxy clusters does not block gravitational waves at the nanohertz frequencies that may be detected by the use of pulsar timing observations.

Authors:
;
Publication Date:
Research Org.:
Univ. of California, San Diego, CA (United States)
Sponsoring Org.:
USDOE Office of Science (SC); National Science Foundation (NSF)
OSTI Identifier:
1530005
Alternate Identifier(s):
OSTI ID: 1611239
Grant/Contract Number:  
de-sc0009919; SC0009919; PHY-1620610
Resource Type:
Published Article
Journal Name:
Physical Review D
Additional Journal Information:
Journal Name: Physical Review D Journal Volume: 99 Journal Issue: 12; Journal ID: ISSN 2470-0010
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Astronomy & Astrophysics; Physics; Gravitation; Gravitational wave detection; Gravitational waves

Citation Formats

Flauger, Raphael, and Weinberg, Steven. Absorption of gravitational waves from distant sources. United States: N. p., 2019. Web. doi:10.1103/PhysRevD.99.123030.
Flauger, Raphael, & Weinberg, Steven. Absorption of gravitational waves from distant sources. United States. https://doi.org/10.1103/PhysRevD.99.123030
Flauger, Raphael, and Weinberg, Steven. Fri . "Absorption of gravitational waves from distant sources". United States. https://doi.org/10.1103/PhysRevD.99.123030.
@article{osti_1530005,
title = {Absorption of gravitational waves from distant sources},
author = {Flauger, Raphael and Weinberg, Steven},
abstractNote = {The rate of gravitational wave absorption by inverse bremsstrahlung is calculated. It increases with decreasing frequency ν as ν–3. Nevertheless, because of the near cancellation of absorption by stimulated emission, the ionized gas in galaxy clusters does not block gravitational waves at the nanohertz frequencies that may be detected by the use of pulsar timing observations.},
doi = {10.1103/PhysRevD.99.123030},
journal = {Physical Review D},
number = 12,
volume = 99,
place = {United States},
year = {Fri Jun 28 00:00:00 EDT 2019},
month = {Fri Jun 28 00:00:00 EDT 2019}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1103/PhysRevD.99.123030

Citation Metrics:
Cited by: 7 works
Citation information provided by
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Works referenced in this record:

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